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19 KiB
19 KiB
1 | ABBR | TERM |
---|---|---|
2 | 21CSLC | 21st Century Space Launch Complex |
3 | 4LGSF | Four-Laser Guide Star Facility |
4 | 4MOST | 4-metre Multi-Object Spectroscopic Telescope (Proposed new spectroscopic instrument for VISTA) |
5 | 4T | Four Telescope (VLTI mode) |
6 | A&A | Journal, Astronomy & Astrophysics |
7 | A&ARv | Journal, Annual Review of Astronomy and Astrophysics |
8 | AAA | Amateur Astronomers Association of New York |
9 | ACD | Amplitude Calibration Device (ALMA) |
10 | ACM | Asteroids, Comets, and Meteors |
11 | ACe | Astaldi Cimolai EIE (Consortium) |
12 | ADA | ALMA Department of Administration |
13 | ADO | ALMA Director’s Office |
14 | ADS | International Italian optics company working on the DSM for the VLT |
15 | AEM | ALMA construction consortium |
16 | AFNOR | Association Française de Normalisation |
17 | AFTA | Astrophysics Focused Telescope Assets |
18 | AGN | Active Galactic Nucleus |
19 | AIDA | Astronomical Infrastructure for Data Access |
20 | AIP | Leibniz Institute for Astrophysics Potsdam |
21 | AIT | Assembly, Integration and Test |
22 | AIV | Assembly, Integration and Verification |
23 | AJ | The Astronomical Journal |
24 | ALMA | Atacama Large Millimeter/submillimeter Array |
25 | AMBER | Astronomical Multi-BEam combineR (VLTI Instrument) |
26 | AN | Journal, Astronomische Nachrichten |
27 | Antu | VLT Unit Telescope 1 |
28 | AO | Adaptive Optics |
29 | AOF | Adaptive Optics Facility |
30 | AOS | Array Operations Site (ALMA) |
31 | APE | Active Phasing Experiment |
32 | APEX | Atacama Pathfinder Experiment |
33 | ApJ | Astrophysical Journal |
34 | ApJS | Journal, Astrophysical Journal Supplement Series |
35 | AQUARIUS | Mid-infrared detector array (VISIR) |
36 | ARAL | Alignment facility for the VLTI |
37 | ARC | ALMA Regional Centre, or Ames Research Center |
38 | ArTeMiS | Bolometric camera for APEX |
39 | ASAC | ALMA Science Advisory Committee |
40 | ASIAA | East Asia FEIC (ALMA) |
41 | ASIC | Application Specific Integrated Circuit |
42 | ASSIST | Adaptive Secondary Setup and Instrument Simulator (AOF test bench) |
43 | AstraLux | Lucky Imaging camera for the Calar Alto 2.2-metre telescope |
44 | AT | Auxiliary Telescope for the VLTI |
45 | ATC | Astronomy Technology Centre (United Kingdom) |
46 | ATILO | Administrative Tribunal of the International Labour Organisation |
47 | AU | Astronomical Unit, the distance between the Earth and the Sun |
48 | AUI | Associated Universities Inc. |
49 | AVM | Astronomical Visualisation Metadata |
50 | AXP | Anomalous X-Ray Pulsar |
51 | BAM | Construction company for the Headquarters extension |
52 | BE | Back-End (ALMA) |
53 | BELLA | Building Europe Link to Latin America |
54 | BFL | Budget and Forward Look |
55 | BH | Black hole |
56 | BLAST | Balloon-borne Large Aperture Submillimeter Telescope |
57 | BlackGEM | (La Silla) Telescope array searching for optical counterparts of gravitational wave sources |
58 | BLIP | Background photon noise limited |
59 | C2PAP | Computational Center for Particle and Astrophysics, Universe Cluster, Garching |
60 | CAD | Computer Aided Design |
61 | CADC | Canadian Astronomy Data Centre |
62 | CAPj | Communicating Astronomy with the Public Journal |
63 | CARLA | Clusters Around Radio-Loud AGN (Spitzer) |
64 | CASA | Common Astronomy Software Applications (ALMA) |
65 | CBR | cosmic background radiation |
66 | CCD | Charge Coupled Device |
67 | CCTV | Closed Circuit TeleVision |
68 | CDR | Critical Design Review |
69 | CDS | Centre de Données astronomiques de Strasbourg (Strasbourg astronomical Data Center) |
70 | CEA | Commissariat à L’Energie Atomique, France |
71 | CELAC_EU | Summit of the Community of Latin American and Caribbean States–European Union |
72 | CES | Coude Echelle Spectrometer |
73 | CfP | Call for Proposal |
74 | CfT | Call for tender |
75 | CGM | Circumgalactic medium |
76 | CHAMP+ | Dual channel heterodyne receiver array (APEX) |
77 | CLIF | Convolution with Linearized Inverse Filter algorithm for wavefront sensing |
78 | CLP | Chilean Peso |
79 | CM | center of mass |
80 | CMB | Cosmic Microwave Background |
81 | CMBR | Cosmic Microwave Background Radiation |
82 | CME | Coronal Mass Ejection (usually Sun) |
83 | CNAM | Conservatoire National des Arts et Métiers |
84 | CNRS | Centre national de la recherche scientifique |
85 | CO | Carbon monoxide |
86 | CO | Carried Over budget |
87 | COFUND | EU fellowship funding programme |
88 | CONDOR | 1.5 THz heterodyne receiver (APEX) |
89 | CONICA | COudé Near-Infrared CAmera (VLT) |
90 | CORALIE | Echelle Spectrograph on the 1.2-metre Leonard Euler Swiss telescope |
91 | CoRoT | COnvection ROtation and planetary Transits (French Satellite) |
92 | COSMOS | HST survey programme |
93 | Cou- | Council Document |
94 | CP | Calibration Programme |
95 | CPI | Consumer Price Index |
96 | CRIRES+ | Planned upgrade to CRIRES |
97 | CRIRES | Cryogenic InfraRed Echelle Spectrometer (VLT) |
98 | CSV | Commissioning and Science Verification |
99 | CTA | Cherenkov Telescope Array |
100 | CTA-S | Cherenkov Telescope Array South |
101 | CTAO | Cherenkov Telescope Array Observatory |
102 | CUBES | Cassegrain U-band Brazilian ESO Spectrograph |
103 | CuRe | Fast wavefront reconstruction algorithms for XAO with pyramid WFS |
104 | CuReD | Fast wavefront reconstruction algorithms for XAO with pyramid WFS with pre-processing |
105 | DC | Direct Current |
106 | DDS | Data DistributIOn middleware for SPARTA |
107 | DDT | Director’s Discretionary Time |
108 | DFG | Deutsche Forschungsgemeinschaft |
109 | DFS | (VLT) Data Flow System |
110 | DG | Director General |
111 | DIG | Deep Imaging Group (Vitacura) |
112 | DL | Delay Line (VLTI) |
113 | DMO | Data Management and Operations Division |
114 | DMS | Dome and Main Structure |
115 | DRS | DRS, formerly Boeing, detector manufacturer |
116 | DSC | Directorate for Science |
117 | DSM | Deformable Secondary Mirror |
118 | DSO | Department of Science Operations (ALMA) |
119 | eAPD | electron Avalanche Photodiode Detector |
120 | EASC | European ALMA Support Centre |
121 | EC | European Commission |
122 | ECRI | European Conference on Research Infrastructures |
123 | EFOSC2 | ESO Faint Object Spectrograph and Camera (v.2) |
124 | EIB | European Investment Bank |
125 | EIROforum | Organisation consisting of the seven largest scientific European international organisations devoted to fostering mutual activities |
126 | ELT | Extremely Large Telescope |
127 | EM&P | Journal, Earth, Moon, and Planets |
128 | EMAC | ELT Management Advisory Committee |
129 | EMBL | European Molecular Biology Laboratory (Germany) |
130 | EMMI | ESO Multi-Mode Instrument (NTT) |
131 | ePOD | education and Public Outreach Department |
132 | ERC | European Research Council |
133 | ERIS | Enhanced Resolution Imager and Spectrograph |
134 | ERP | Enterprise Resource Planning (Administration software) |
135 | ESAC | European Science Advisory Committee (for ALMA) |
136 | ESAC | European Space Astronomy Centre (ESA, Spain) |
137 | ESC | ELT Subcommittee |
138 | ESE | ELT Science and Engineering |
139 | ESM | European School Munich |
140 | ESO | European Organisation for Astronomical Research in the Southern Hemisphere |
141 | ESOF | Euroscience Open Forum |
142 | ESON | ESO Science Outreach Network |
143 | ESPRESSO | Echelle SPectrograph for Rocky Exoplanet- and Stable Spectroscopic Observations |
144 | ESRC | ELT Standing Review Committee |
145 | ETF | ELT Technical Facility |
146 | EVALSO | Enabling Virtual Access to Latin-american Southern Observatories |
147 | EWASS | European Week of Astronomy and Space Science |
148 | ExA | Journal, Experimental Astronomy |
149 | ExTrA | (La Silla) Exoplanets in Transit and their Atmospheres |
150 | FC | Finance Committee |
151 | FDR | Final Design Review |
152 | FE IPT | Front-End Integrated Project Team (ALMA) |
153 | FE | Front End |
154 | FEA | Finite Element Analysis |
155 | FEED | Front-End Engineering Design (ELT) |
156 | FEIC | Front End Integration Centre (ALMA) |
157 | FEROS | Fibre-fed, Extended Range, Échelle Spectrograph (MPG/ESO 2.2-metre) |
158 | FIAT | Facility (for) Infrared Arrays Testing |
159 | FITS | Flexible Image Transport System |
160 | FLAMES | Fibre Large Array Multi Element Spectrograph (VLT) |
161 | FORS1 | FOcal Reducer/low dispersion Spectrograph (VLT)-1 |
162 | FORS2 | FOcal Reducer/low dispersion Spectrograph (VLT)-2 |
163 | FOS | Faint Object Spectrograph (HST) |
164 | FP | Fabry-Perot |
165 | FP6 | Sixth EC Framework Programme |
166 | FP7 | Seventh EC Framework Programme |
167 | FWHM | Full Width at Half Maximum |
168 | GALACSI | Ground Atmospheric Layer Adaptive Optics for Spectroscopic Imaging (AOF) |
169 | GIRAFFE | Fibre-fed multi-object spectrograph and part of the VLT FLAMES facility |
170 | GLAO | Ground Layer Adaptive Optics |
171 | gNLT | Garching Night Log Tool |
172 | GRAAL | GRound-layer Adaptive optics Assisted by Lasers (AOF) |
173 | GRAVITY | AO assisted, two-object, multiple-beam-combiner (VLTI) |
174 | GROND | Gamma-Ray Burst Optical/Near-Infrared Detector (MPG/ESO 2.2-metre) |
175 | GTC | Gran Telescopio Canarias |
176 | GTO | Guaranteed Time for Observation |
177 | GWh | Gigawatt hours |
178 | GÉANT | European multi-gigabit computer network for research and education purposes |
179 | H-LTAO | HARMONI Laser Tomography Adaptive Optics |
180 | H2020 | (EU) Horizon 2020 Programme |
181 | HARMONI | Proposed first light integral field spectrograph for the ELT |
182 | HARPS | High Accuracy Radial Velocity Planetary Searcher (3.6-metre) |
183 | HAWK-I | High Acuity Wide field K-band Imager |
184 | HCI | Human Computer Interface |
185 | HIA | Herzberg Institute of Astrophysics (Canada) |
186 | HIRES | (ELT) HIgh REsolution Spectrograph |
187 | HODM | High Order Deformable Mirror |
188 | HST | Hubble Space Telescope |
189 | HVAC | Heating, Ventilation and Air Conditioning |
190 | IAG | Institute of Astronomy, Geophysics and Atmospheric Sciences (Brazil) |
191 | IAS | International Accounting Standards |
192 | IAU | International Astronomical Union |
193 | Icar | Icarus, Planetary science journal, Planetary science journal |
194 | IFS | Integral Field Spectrograph (SPHERE, ELT) |
195 | IFU | Integral Field Unit |
196 | INAF | Italian National Institute for Astrophysics |
197 | INRIA | Institut National de Recherche en Informatique et en Automatique |
198 | IPAG | Institut de Planetologie et d’Astrophysique de Grenoble |
199 | IPC | (Chilean) Índice de Precios al Consumidor |
200 | IPP | Max-Planck Institute for Plasma Physics (Germany) |
201 | IPSAS | International Public Sector Accounting Standards |
202 | IPT | Integrated Product Team (ALMA) |
203 | IR | Infrared |
204 | IRAM | Institut de Radioastronomie Millimétrique |
205 | IRDIS | InfraRed Dual-beam Imager and Spectrograph (SPHERE, ELT) |
206 | IRIS | VLTI Infrared Image Sensor |
207 | IRLOS | InfraRed Low Order Sensor |
208 | IRO | International Relations Office |
209 | ISAAC | Infrared Spectrometer And Array Camera (VLT) |
210 | ISERD | Israeli inter-ministerial agency for R&D cooperation with Europe |
211 | ISM | International Staff Member |
212 | ISS | International Space Station |
213 | IT | Information Technology |
214 | ITAR | International Traffic in Arms Regulations |
215 | ITER | International Thermonuclear Experimental Reactor |
216 | IVOA | International Virtual Observatory Alliance |
217 | IVSLA | Istituto Veneto di Scienze ed Arti |
218 | IYA2009 | International Year of Astronomy 2009 |
219 | JAO | Joint ALMA Observatory |
220 | JENAM | Joint European and National Astronomy Meeting |
221 | JPL | Jet Propulsion Laboratory |
222 | JUICE | JUpiter ICy moons Explorer |
223 | JWST | James Webb Space Telescope |
224 | k | kilo/1,000 |
225 | KIDS | (VST) Kilo-Degree Survey |
226 | KMOS | K-band Multi-Object Spectrograph (VLT) |
227 | KTS | Klaus Tschira Stiftung |
228 | Kueyan | VLT Unit Telescope 2 |
229 | LABOCA | Large APEX Bolometer CAmera |
230 | LAOG | Laboratoire d'Astrophysique de l'Observatoire de Grenoble |
231 | LCS | Local Control System |
232 | LEO | Low Earth Orbit |
233 | LFC | Laser Frequency Comb |
234 | LGS | Laser Guide Star |
235 | LGSF | Laser Guide Star Facility |
236 | LMC | Large Magellanic Cloud |
237 | LMU | Ludwig-Maximilians-Universität München |
238 | LN2 | Liquid nitrogen |
239 | LOFAR | Low Frequency Array |
240 | LOPS | Local Optical Phasing Sensor |
241 | LP | Large Programme |
242 | LPG | Liquefied Petroleum Gas |
243 | LPO | La Silla Paranal Observatory |
244 | LSM | Local Staff Members |
245 | LSP | La Silla Paranal Subcommittee |
246 | LTAO | Laser Tomography Adaptive Optics |
247 | LVSM | Large Visible Sensor Module |
248 | M# | Mirror # |
249 | M | million/1,000,000 |
250 | MACAO | Multiple Application Curvature Adaptive Optic |
251 | MACCON | Motion controller manufacturer |
252 | MAD | Multi-conjugate Adaptive optics Demonstrator |
253 | MAORY | (ELT) Multi-conjugate Adaptive Optics RelaY |
254 | mas | milliarcseconds |
255 | MASCOT | Mini All-Sky Cloud Observation Tool (Paranal) |
256 | MATISSE | Multi AperTure mid-Infrared SpectroScopic Experiment (VLTI) |
257 | MCAO | Multi-Conjugate Adaptive Optics |
258 | Melipal | VLT Unit Telescope 3 |
259 | MELT | Minuscule ELT |
260 | MENLO systems | Optical equipment manufacturer |
261 | MERAC | Mobilising European Research in Astrophysics and Cosmology |
262 | MERIL | Mapping the European Research Infrastructure Landscape |
263 | METIS | Mid-infrared ELT Imager and Spectrograph |
264 | MICADO | Adaptive optics imaging camera (ELT) |
265 | MIDI | Mid-infrared Interferometric Instrument (VLTI) |
266 | MIM | Museo Interactivo Mirador, Santiago |
267 | MIT | Massachusetts Institute of Technology |
268 | mmVLBI | Millimeter Very Long Baseline Interferometry |
269 | Mn | Mirror #n |
270 | MNRAS | Journal, Monthly Notices of the Royal Astronomical Society |
271 | MOAO | Multiple-Object Adaptive Optics |
272 | MOONS | Multi Object Optical and Near-infrared Spectrograph (VLT third generation) |
273 | MOS | (ELT) Multi-Object Spectroscopy |
274 | MOSAIC | (ELT) Multi-Object Spectrograph (Multi-Object Spectrograph for Astrophysics, Intergalactic medium studies and Cosmology) |
275 | MOSFIRE | Near-infrared multi-object spectrograph (Keck) |
276 | MPA | Max Planck Institute for Astrophysics |
277 | MPE | Max Planck Institute for Extraterrestrial Physics |
278 | MPG | Max-Planck-Gesellschaft |
279 | MPIA | Max Planck Institute for Astronomy |
280 | MPIfR | Max-Planck Institute for Radioastronomy (Germany) |
281 | MS | Member State(s) |
282 | MTM | MT Mechatronics (European company of high technology, engineering and maintenance services) |
283 | MUSE | Multi Unit Spectroscopic Explorer (VLT) |
284 | NACO | NAOS-CONICA (VLT) |
285 | NAOJ | National Astronomical Observatory of Japan |
286 | NAOMI | Adaptive optics system for the ATs (VLTI) |
287 | NAOS | Nasmyth Adaptive Optics System (VLT) |
288 | NASA | National Aeronautics and Space Administration |
289 | NAV | Navision |
290 | NDF | Non-Deliverable Forward Agreement |
291 | NEAR | New Earths in the Alpha Cen Region experiment |
292 | NEO | Near-Earth Object |
293 | NewA | Journal, New Astronomy |
294 | NewAR | Journal, New Astronomy Reviews |
295 | NFM | Narrow Field Mode |
296 | NGC | New General Catalogue |
297 | NGC | New General detector Controller |
298 | NGSD | Proposed large natural/laser guide star WFS detector (ELT) |
299 | NGTS | Next Generation Transit Survey |
300 | NINS | National Institutes of Natural Sciences |
301 | NIRPS | (NNT) Near Infra Red Planet Searcher |
302 | NOVA | The Netherlands Research School for Astronomy (Nederlandse Onderzoekschool voor Astronomie) |
303 | NRAO | National Radio Astronomy Observatory |
304 | NSF | National Science Foundation |
305 | NTT | New Technology Telescope |
306 | NUVA | Network for UltraViolet Astrophysics |
307 | OAA | Arcetri Astrophysical Observatory |
308 | OBAMA | Optical Bidule for Aberration Measurement on the ATs |
309 | OCA-NICE | Cote d’Azur Observatory (Observatoire de la Cote d’Azur) |
310 | ODG | Office of the Director General |
311 | OECD | Organisation for Economic Co-operation and Development |
312 | OmegaCAM | Optical Camera for the VST |
313 | OPC | Observing Programmes Committee |
314 | OPO | Observing Programmes Office |
315 | OPTICON | Optical Infrared Coordination Network for Astronomy |
316 | OSF | ALMA Operations Support Facilities |
317 | OSO | Onsala Space Observatory |
318 | OT | Observing Tool |
319 | OTS | Operations Technical Support |
320 | P&SS | Journal, Planetary and Space Science |
321 | P2PP | Peer to Peer Protocol |
322 | P86 | Observing Period 86 |
323 | P87 | Observing Period 87 |
324 | PA | Product Assurance |
325 | PAC | Provisional Acceptance Chile |
326 | PACMAN | Fringe tracker for PRIMA (VLTI) |
327 | PAE | Provisional Acceptance Europe |
328 | PARLA | PAranal Raman Laser, replacement for PARSEC (VLTI) |
329 | PARSEC | Sodium line laser for VLT AO |
330 | PASJ | Journal, Publications of the Astronomical Society of Japan |
331 | PASP | Journal, Publications of the Astronomical Society of the Pacific |
332 | PDR | Preliminary Design Review |
333 | PESSTO | Public ESO Spectroscopic Survey of Transient Objects |
334 | PFS | (ELT) Pre-Focal Station |
335 | PFS-A | (ELT) Pre-Focal Station for Nasmyth A |
336 | PhD | Doctor of Philosophy |
337 | PI | Principal Investigator |
338 | PIO | Public Information Officer |
339 | PIONIER | VLTI visitor instrument |
340 | PIP | Paranal Instrumentation Programme |
341 | PLC | Programmable Logic Controllers (ELT) |
342 | PMD | Project Management Department |
343 | PMPD | Performance Management and Professional Development |
344 | PRIMA | Phase-Referenced Imaging and Micro-arcsecond Astrometry facility (VLTI) |
345 | PSF | Point Spread Function |
346 | PTP | Precision Time Protocol |
347 | Q | Quarter |
348 | QSO | Quasi Stellar Object, quasar |
349 | QUEST | QUasar Equatorial Survey Team |
350 | R&D | Research and Development |
351 | RAB | Reflector Assembly Building |
352 | RAL | Rutherford Appleton Laboratory, Didcot (UK) |
353 | RCL | Radioastronomy Chajnantor Limitada |
354 | RedCLARA | Latin American Advanced Networks Cooperation (Academic data network in Latin America) |
355 | REM | Rapid Eye Mount Telescope (La Silla) |
356 | REUNA | Red Universitaria Nacional (Academic data network in Chile) |
357 | RM | Rossiter-McClaughlin (effect) |
358 | RMN | Reflective Memory Network (VLTI) |
359 | rms | Root Mean Square |
360 | SABOCA | Shortwave Apex BOlometer Camera |
361 | SAC | EURO-VO Science Advisory Committee |
362 | SAF | Science Archive Facility |
363 | SAFRAN-REOSC | High performance optics company |
364 | SAPHIRA | Detector for the GRAVITY wavefront sensor |
365 | SAXO | SPHERE’S AO system (VLT) |
366 | SCAO | Single-conjugate adaptive optics |
367 | SCO | Santiago Central Office (ALMA/ESO Vitacura) |
368 | SDD | Software Development Division |
369 | SDSS | Sloan Digital Sky Survey |
370 | SEPIA | Swedish ESO PI receiver for APEX |
371 | SHFI | Swedish Heterodyne Facility Instrument |
372 | SiC | (ELT) SiliconCarbide-mirrorsubstrate |
373 | SINFONI | Spectrograph for INtegral Field Observations in the Near Infrared (VLT) |
374 | SKA | Square Kilometer Array |
375 | SM | Service Mode (observing) |
376 | SM4 | Servicing Mission 4 (HST) |
377 | SMBH | Supermassive black hole |
378 | SOFI | SOn oF Isaac (NTT) |
379 | SOPHIE | Spectrographe pour l’Observation des Phénomènes des Intérieurs stellaires et des Exoplanètes |
380 | SOXS | (NTT) Son Of X-Shooter |
381 | SPARTA | Real-time computer for the AOF |
382 | SPC | Scientific Personnel Committee |
383 | SPECULOOS | (Paranal) Search for habitable Planets EClipsing ULtra-cOOl Stars |
384 | SPHERE | Spectro-Polarimetric High-contrast Exoplanet Research instrument (VLT) |
385 | SPIFFI | SPectrometer for Infrared Faint Field Imaging |
386 | SPT | South Pole Telescope |
387 | SSDF | Science Support Discretionary Fund |
388 | SSED | Software System Engineering Department |
389 | SSWG | Science Strategy Working Group |
390 | ST-ECF | Space Telescope European Coordination Facility |
391 | STC | Scientific Technical Committee |
392 | STFC | Science and Technology Facilities Council (UK) |
393 | STRAP | Tip-tilt sensors (VLTI) |
394 | STScI | Space Telescope Science Institute (USA) |
395 | sub-mm | submillimetre |
396 | SUSI2 | Superb Seeing Imager 2 (NTT) |
397 | TAROT | Télescope à Action Rapide pour les Objets Transitoires |
398 | TAROT-S | Télescopes à Action Rapide pour les Objets Transitoires South |
399 | TBT | Test-Bed Telescope |
400 | TEC | Technology Division |
401 | telbib | ESO library telescope bibliography database |
402 | TFB | Tunable Filter Bank (ALMA) |
403 | TIMMI | TIMMI far-infrared camera (ESO 3.6-metre telescope) |
404 | ToO | Target of Opportunity |
405 | TRAPPIST | TRAnsiting Planets and PlanetesImals Small Telescope |
406 | TRR | Test Readiness Review |
407 | TUM | Technische Universität München |
408 | UC | Users Committee |
409 | UK ATC | UK Astronomy Technology Centre |
410 | Ultracam | High-speed camera (VLT) |
411 | UltraVISTA | Ultra-deep near-infrared survey in the COSMOS field |
412 | UNCOPUOS | United Nations Committee for the Peaceful Uses of Outer Space |
413 | USM | University Observatory Munich |
414 | UT | Unit Telescope of the VLT |
415 | UT1–4 | VLT Unit Telescopes 1–4: Antu, Kueyen, Melipal and Yepun |
416 | UV | UltraViolet |
417 | UVES | UV-Visual Echelle Spectrograph (VLT) |
418 | VAT | Value Added Tax |
419 | VERTEX | (APEX) VERTEX Antennentechnik GmbH, Duisburg (Germany) |
420 | VHS | VISTA Hemisphere Survey |
421 | VIDEO | VISTA Deep Extragalactic Observations Survey |
422 | VIKING | VISTA Kilo-degree Infrared Galaxy survey |
423 | VIMOS | VIsible MultiObject Spectrograph (VLT) |
424 | VINCI | VLT INterferometer Commissioning Instrument (VLTI) |
425 | VIPERS | VIMOS Public Extragalactic Redshift Survey |
426 | VIRCAM | VISTA Infrared Camera |
427 | VISA | VLTI Sub-Array |
428 | VISIR | VLT Mid-Infrared Imager Spectrometer |
429 | VISTA | Visible and Infrared Survey Telescope for Astronomy |
430 | VLT | Very Large Telescope |
431 | VLT/I | Very Large Telescope and its Interferometer |
432 | VLTI | Very Large Telescope Interferometer |
433 | VLTI-PR# | VLTI projects |
434 | VM | Visitor Mode (observing) |
435 | VMC | VISTA survey of the Magellanic Cloud system |
436 | VO | Virtual Observatory |
437 | VOP | Virtual Observatory Project Office |
438 | VPHAS+ | VST Photometric Hα Survey |
439 | VSS | Variability Sky Survey |
440 | VST | VLT Survey Telescope |
441 | VVDS | VIMOS VLT Deep Survey |
442 | VVV | ESO public survey VISTA Variables in the Vía Láctea |
443 | WASP | Wide Angle Search for Planets survey |
444 | WFCAM | Infrared wide field camera for the UK Infrared Telescope on Mauna Kea |
445 | WFI | Wide Field Imager (MPG/ESO 2.2-metre) |
446 | WiFi | Wireless Fidelity |
447 | WVR | Water Vapour Radiometer (ALMA) |
448 | X-shooter | Wideband ultraviolet-infrared single target spectrograph (VLT) |
449 | XAO | Extreme adaptive optics |
450 | XMM-Newton | X-ray Multi-Mirror satellite (ESA) |
451 | Yepun | VLT Unit Telescope 4 |
452 | Z-Spec | Millimetre-wave spectrograph (APEX visitor instrument) |
453 | zCOSMOS | Large Programme to measure 30 000 galaxies in the HST Cosmic Origins field |
454 | ZIMPOL | Zurich Imaging Polarimeter (SPHERE, ELT) |
455 | ΛCDM | Lambda Cold Dark Matter |
456 | μm | Micrometre |